Kim Venn

Professor

University of Victoria

Canada

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Professor Kim Venn is a faculty member at the University of Victoria, Canada. Her research focuses on the chemodynamics of Milky Way satellites, stellar populations in dwarf galaxies, and advanced photometric techniques. Recent publications include studies on extremely metal-poor stars and their role in early galactic assembly, as well as analyses of globular cluster morphology and stellar haloes.

Kim Venn

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Articles (20)

GHOST Commissioning Science Results. IV. Chemodynamical Analyses of Milky Way Satellites Sagittarius II and Aquarius II

ACACIAS I: element abundance labels for 192 stars in the dwarf galaxy NGC 6822

C-19 and Hot, Wide Star Streams

Accreted globular clusters and horizontal branch morphology in the outer halo of M31

Pushing the limits of near-infrared photometry with the Gemini Multi-Conjugate Adaptive Optics System: study of crowded fields in the globular cluster M5

GHOST commissioning science results – II: a very metal-poor star witnessing the early galactic assembly

GHOST Commissioning Science Results: Identifying a New Chemically Peculiar Star in Reticulum II

The extended ‘stellar halo’ of the Ursa Minor dwarf galaxy

StarUnLink: identifying and mitigating signals from communication satellites in stellar spectral surveys

The Pristine Inner Galaxy Survey (PIGS) VII: a discovery of the first inner Galaxy CEMP-r/s star

Stars on the edge: Galactic tides and the outskirts of the Sculptor dwarf spheroidal

SPLUS J142445.34–254247.1: An r-process–enhanced, Actinide-boost, Extremely Metal-poor Star Observed with GHOST

Probing the early Milky Way with GHOST spectra of an extremely metal-poor star in the Galactic disc

Small-scale stellar haloes: detecting low surface brightness features in the outskirts of Milky Way dwarf satellites

The Pristine survey – XXII. A serendipitous discovery of an extremely Li-rich very metal-poor giant and a new method of 6Li/7Li isotope measurement

The Cosmic Hunt for members in the outskirts of ultra-faint dwarf galaxies: Ursa Major I, Coma Berenices, and Boötes I

The Pristine Inner Galaxy Survey (PIGS) – V. A chemo-dynamical investigation of the early assembly of the Milky Way with the most metal-poor stars in the bulge

The Pristine survey – XVII. The C-19 stream is dynamically hot and more extended than previously thought

Optimal Differential Astrometry for Multiconjugate Adaptive Optics. I. Astrometric Distortion Mapping using On-sky GeMS Observations of NGC 6723

The Pristine survey – XV. A CFHT ESPaDOnS view on the Milky Way halo and disc populations

Collaborators (9)

Jon Lawrence

Julio Navarro

Richard McDermid

Vinicius Placco

Amanda Karakas

Simon Smith

Carmela Lardo

Melissa Ness

Zhen Yuan

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